The collision-induced absorption of H2 near 1.20 μm: Subatmospheric measurements and validation tests of calculations

被引:1
|
作者
Koroleva, A. O. [1 ,2 ]
Kassi, S. [1 ]
Fleurbaey, H. [1 ]
Campargue, A. [1 ]
机构
[1] Univ Grenoble Alpes, CNRS, LIPhy, F-38000 Grenoble, France
[2] Russian Acad Sci, AV Gaponov Grekhov Inst Appl Phys, 46 Ulyanov Str, Nizhnii Novgorod 603950, Russia
关键词
Collision-induced absorption; Molecular hydrogen; CIA; Absorption continua; H2; INDUCED INFRARED-SPECTRUM; 2ND OVERTONE BAND; INTERCOLLISIONAL INTERFERENCE; RAYLEIGH-SCATTERING; CAVITY RING; H-2; PAIRS; HYDROGEN; 1ST; TEMPERATURES; H-2-H-2;
D O I
10.1016/j.jqsrt.2024.108948
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
The weak binary collision -induced absorption (CIA) of molecular hydrogen is measured at room temperature in the first overtone region near 1.20 mu m. Binary absorption coefficients are derived by cavity ring down spectroscopy (CRDS) at 28 selected spectral points sampling the (2-0) band between 7974 and 8650 cm -1. While all previous studies used high density samples, the sensitivity of the CRDS method allowed deriving accurate CIA by using pressure ramps of pure H2 limited to a maximum pressure of 1 atm. After subtraction of the Rayleigh contribution, a purely quadratic pressure dependence is obtained for the absorption coefficient at each measurement point and the CIA binary coefficients are derived with a 1.5 % accuracy. The comparison to theoretical values widely used for astronomical applications shows deviations values between 5 and 25 %.
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页数:6
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